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Physical Processes in Solar Flares

Physical Processes in Solar Flares

Hardcover

Series: Astrophysics and Space Science Library, Book 172

Astronomy & SpacePhysics

ISBN10: 0792312619
ISBN13: 9780792312611
Publisher: Springer Nature
Published: Dec 31 1991
Pages: 249
Weight: 1.25
Height: 0.81 Width: 6.48 Depth: 9.54
Language: English
Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects.
This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets.
The author believes that this model will help to solve the problem of solar flares.
For solar physicists, plasma physicists, high-energy particle physicists.

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